10th Meeting

Wednesday 30 Sept 2020, 12:00 → 13:00 US/Eastern

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https://bluejeans.com/771188806?src=join_info

Meeting ID
771 188 806

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12:00 → 12:30 Update on complementarity from the Far Forward and IR WG group

Questions to start discussion:

• What is your current baseline thinking?

• How might a second detector differ in technology choices and what (dis)advantages might that bring in terms of kinematic coverage, resolution on reconstructed variables, radiation hardness, dominating systematics etc?

  • Are there wider implications for other parts of the detector - eg due to material budgets?

  • Would the complementary designs naturally be associated with different choices of solenoid field, centre of mass energy, luminosity or beam polarisation?

  • Are there any limitations in the performance of your sub detector technologies for very small bunch spacing < 9ns

  • Are there any rate limitations?

  • Is +/- 4.5 m enough longitudinal space to fit the detector

  • Are there any issues we should be aware of in terms of cost, technology readiness, or time required to construct the detector?

  • Might it be possible to combine more than one function into your detector(s)?

  • Do your detector technologies have any impact on the design of the interaction region?

  • What studies need to be done (or have been done already) to make fully quantitative statements?

Speakers: Alexander Jentsch (Brookhaven National Lab), Yulia Furletova (Jefferson Lab)

FF_Complementarity_Meeting_9_30_2020_v1.pdf

FF_Complementarity_Meeting_9_30_2020_v1.pptx